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Model Atmospheres of Be Stars

Published online by Cambridge University Press:  14 August 2015

Roland Poeckert
Roland Poeckert*
Affiliation:
Dominion Astrophysical Observatory, Herzberg Institute of Astrophysics, Victoria, B.C.

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The basic concept of what a Be star is we owe to Struve (1931). His proposal that these stars are rapidly rotating and have an extended, disc-like, circumstellar envelope is still the basis for all models of Be stars. Unfortunately, progress in understanding the dynamics of Be stars has been painfully slow, a consequence of the very complex nature of the problem. As yet there does not exist a self-consistent unique model of any Be star.

Type
VIII. Atmospheric Models
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 453 - 483
Copyright
Copyright © Reidel 1982 

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